Search results for " Dynamics"

showing 10 items of 4108 documents

Understanding social behavior evolutions through agent-based modeling

2012

Agent-based social simulation as a computational approach to social simulation has been largely used to explore social phenomena. The purpose of this paper is to describe a theoretical model of transmission and evolution of social behaviors in a network of artificial societies (artificial world) using agent-based modeling technology. In this model, each agent (society) is subdivided into social behaviors where individual and social learning occur. The agent-agent interactions are carried out by their social behaviors; otherwise the agent-environment interactions through consumption of ecological resources by its social behaviors in repression and satisfaction. We distinguish social behavior…

Artificial worldSocial dynamicsGlobalizationManagement scienceComputer sciencebusiness.industryMulti-agent systemArtificial intelligencebusinessSocial learningSocial heuristicsSocial behaviorSocial simulation2012 International Conference on Multimedia Computing and Systems
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MOJAVE. XII. ACCELERATION AND COLLIMATION OF BLAZAR JETS ON PARSEC SCALES

2014

We report on the acceleration properties of 329 features in 95 blazar jets from the MOJAVE VLBA program. Nearly half the features and three-quarters of the jets show significant changes in speed and/or direction. In general, apparent speed changes are distinctly larger than changes in direction, indicating that changes in the Lorentz factors of jet features dominate the observed speed changes rather than bends along the line of sight. Observed accelerations tend to increase the speed of features near the jet base, $\lesssim 10-20$ parsecs projected, and decrease their speed at longer distances. The range of apparent speeds at fixed distance in an individual jet can span a factor of a few, i…

AstrofísicaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencessymbols.namesakeAcceleration0103 physical sciencesBlazar010303 astronomy & astrophysicsVery Long Baseline ArrayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Line-of-sightShock (fluid dynamics)010308 nuclear & particles physicsAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxyLorentz factorSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)AstronomiasymbolsAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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Efficient generation of energetic ions in multi-ion plasmas by radio-frequency heating

2017

We describe a new technique for the efficient generation of high-energy ions with electromagnetic ion cyclotron waves in multi-ion plasmas. The discussed ‘three-ion’ scenarios are especially suited for strong wave absorption by a very low number of resonant ions. To observe this effect, the plasma composition has to be properly adjusted, as prescribed by theory. We demonstrate the potential of the method on the world-largest plasma magnetic confinement device, JET (Joint European Torus, Culham, UK), and the high-magnetic-field tokamak Alcator C-Mod (Cambridge, USA). The obtained results demonstrate efficient acceleration of 3He ions to high energies in dedicated hydrogen–deuterium mixtures.…

Astrophysical plasmasTokamakradio-frequency heatingCyclotronJoint European TorusPlasma heatingGeneral Physics and AstronomyFREQUENCY114 Physical sciences01 natural sciences7. Clean energyMagnetically confined plasmas010305 fluids & plasmaslaw.inventionIonPHYSICSPhysics and Astronomy (all)FUSIONMODE CONVERSIONlawPhysics::Plasma Physics0103 physical sciencesDielectric heating010306 general physicsPhysics[PHYS]Physics [physics]ta114Solar flare:Física [Àrees temàtiques de la UPC]Plasma dynamicsmulti-ion plasmasSettore FIS/01 - Fisica SperimentaleMagnetic confinement fusionPlasmaHE-3-RICH SOLAR-FLARESTècniques de plasmaJETCYCLOTRON RANGETOKAMAKPhysics::Space PhysicsAtomic physicsHE-3-RICH SOLAR-FLARES; MODE CONVERSION; CYCLOTRON RANGE; FUSION; JET; FREQUENCY; TOKAMAK; PHYSICS
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History and results of the Riga dynamo experiments

2008

On 11 November 1999, a self-exciting magnetic eigenfield was detected for the first time in the Riga liquid sodium dynamo experiment. We report on the long history leading to this event, and on the subsequent experimental campaigns which provided a wealth of data on the kinematic and the saturated regime of this dynamo. The present state of the theoretical understanding of both regimes is delineated, and some comparisons with other laboratory dynamo experiments are made.

Astrophysics (astro-ph)Fluid Dynamics (physics.flu-dyn)General EngineeringFOS: Physical sciencesEnergy Engineering and Power TechnologyChamp magnetiqueGeophysicsPhysics - Fluid DynamicsAstrophysicsPhysics::GeophysicsPhysics::Fluid DynamicsNuclear magnetic resonanceDynamo theoryMagnetohydrodynamicsGeologyDynamo
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Effects of radiation in accretion regions of classical T Tauri stars

2019

Models and observations indicate that the impact of matter accreting onto the surface of young stars produces regions at the base of accretion columns, in which optically thin and thick plasma components coexist. Thus an accurate description of these impacts requires to account for the effects of absorption and emission of radiation. We study the effects of radiation emerging from shock-heated plasma in impact regions on the structure of the pre-shock downfalling material. We investigate if a significant absorption of radiation occurs and if it leads to a pre-shock heating of the accreting gas. We developed a radiation hydrodynamics model describing an accretion column impacting onto the su…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsradiation: dynamics01 natural sciencesaccretion0103 physical sciencesThermalRadiative transferAstrophysics::Solar and Stellar Astrophysics010306 general physicsAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsultraviolet: starsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsstars: variables: T Tauristars: formationaccretion disksHerbig Ae/BeAstronomy and AstrophysicsPlasmaThermal conductionAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomena
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ASYMPTOTIC ANALYSIS OF THE LINEARIZED NAVIER–STOKES EQUATION ON AN EXTERIOR CIRCULAR DOMAIN: EXPLICIT SOLUTION AND THE ZERO VISCOSITY LIMIT

2001

In this paper we study and derive explicit formulas for the linearized Navier-Stokes equations on an exterior circular domain in space dimension two. Through an explicit construction, the solution is decomposed into an inviscid solution, a boundary layer solution and a corrector. Bounds on these solutions are given, in the appropriate Sobolev spaces, in terms of the norms of the initial and boundary data. The correction term is shown to be of the same order of magnitude as the square root of the viscosity. Copyright © 2001 by Marcel Dekker, Inc.

Asymptotic analysisApplied MathematicsMathematical analysisAsymptotic analysis; Boundary layer; Explicit solutions; Navier-Stokes equations; Stokes equations; Zero viscosity; Mathematics (all); Analysis; Applied MathematicsMathematics::Analysis of PDEsAnalysiStokes equationDomain (mathematical analysis)Navier-Stokes equationPhysics::Fluid DynamicsSobolev spaceAsymptotic analysiBoundary layersymbols.namesakeBoundary layerSquare rootExplicit solutionInviscid flowStokes' lawsymbolsMathematics (all)Zero viscosityNavier–Stokes equationsAnalysisMathematicsCommunications in Partial Differential Equations
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Monsoon Multidisciplinary Analysis (AMMA) : an integrated project for understanding of the West African climate system and its human dimension

2011

International audience; The intraseasonal time scale is critical in West Africa where resources are highly rainfall dependent. Three main modes of variability have been identified, two with a mean periodicity of 15 days and one with a mean periodicity around 40 days. These modes have a regional scale and can strongly influence precipitation and convective activity. They are mainly controlled by atmospheric dynamics and land-surface interactions. They can also modulate the very specific phase of the African summer monsoon onset. A better knowledge of the mechanisms controlling this scale is necessary to improve its predictability.

Atmospheric Science010504 meteorology & atmospheric sciences0207 environmental engineering02 engineering and technology[SDU.STU.ME]Sciences of the Universe [physics]/Earth Sciences/MeteorologyIntraseasonal variabilityMonsoonAtmospheric sciences01 natural sciencesWest africaWest African monsoonpredictabilityMonsoon onsetmonsoon onsetCrop yieldPrecipitationPredictability020701 environmental engineering0105 earth and related environmental sciencesintraseasonal variability[ SDU.STU.ME ] Sciences of the Universe [physics]/Earth Sciences/Meteorologycrop yieldScale (music)PredictabilityWest african13. Climate actionClimatologyEnvironmental scienceAtmospheric dynamics
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Sun-Earth System Interaction studies over Vietnam: an international cooperative project

2006

International audience; During many past decades, scientists from various countries have studied separately the atmospheric motions in the lower atmosphere, in the Earth's magnetic field, in the magnetospheric currents, etc. All of these separate studies lead today to the global study of the Sun and Earth connections, and as a consequence, new scientific programs (IHY- International Heliophysical Year, CAWSES- Climate and Weather in the Sun-Earth System) are defined, in order to assume this new challenge. In the past, many scientists did not have the possibility to collect data at the same time in the various latitude and longitude sectors. Now, with the progress of geophysical sciences in …

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorology[SDE.MCG]Environmental Sciences/Global ChangesContext (language use)Monsoon01 natural sciences[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/Climatology0103 physical sciencesEarth and Planetary Sciences (miscellaneous)lcsh:Science010303 astronomy & astrophysicsdiurnal to secular)0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmospherelcsh:QC801-809GeologyAstronomy and AstrophysicsEquatorial electrojetOrographylcsh:QC1-999International Heliophysical YearIonosphere (Electric fields and currents)lcsh:Geophysics. Cosmic physics[SDE.MCG] Environmental Sciences/Global Changes[ SDE.MCG ] Environmental Sciences/Global ChangesGeography13. Climate actionSpace and Planetary Science[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyGeomagnetism and paleomagnetism (Time variationsMeteorology and dynamics (Tropical meteorology)lcsh:QTropical cycloneIonosphere[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyLongitudelcsh:Physics
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The Role of Wind Speed and Wind Shear for Banner Cloud Formation

2019

Abstract Banner clouds are clouds that appear to be attached to the leeward face of a steep mountain. This paper investigates the role of wind speed and wind shear for the formation of banner clouds. Large-eddy simulations are performed to simulate the flow of dry air past an idealized pyramid-shaped mountain. The potential for cloud formation is diagnosed through the Lagrangian vertical parcel displacement, which in the case of a banner cloud shows a plume of large values in the lee of the mountain. In addition, vortical structures are visualized through streamlines and their curvature. A series of sensitivity experiments indicates that both the flow and the banner cloud occurrence are lar…

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorologybusiness.industryCloud computing010501 environmental sciences01 natural sciencesVertical motionWind speedPhysics::Fluid DynamicsAtmosphereBoundary layerWind shearBannerbusinessPhysics::Atmospheric and Oceanic PhysicsGeology0105 earth and related environmental sciencesJournal of the Atmospheric Sciences
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The Effect of Turbulence on the Accretional Growth of Graupel

2019

Abstract Wind tunnel experiments were carried out to investigate the influence of turbulence on the collection kernel of graupel. The collection kernel defines the growth rate of a graupel accreting supercooled droplets as it falls through a cloud. The ambient conditions were similar to those occurring typically in the mixed-phase zone of convective clouds, that is, at temperatures between −7° and −16°C and with liquid water contents from 0.5 to 1.3 g m−3. Tethered spherical collectors with radii between 220 and 340 μm were exposed in a flow carrying supercooled droplets with a mean volume radius of 10 μm. The vertical root-mean-square fluctuation velocity, the dissipation rate, and the Tay…

Atmospheric Science010504 meteorology & atmospheric sciencesTurbulence01 natural sciences010305 fluids & plasmasPhysics::Fluid DynamicsKernel (statistics)0103 physical sciencesGrowth ratePrecipitationStatistical physicsGraupel0105 earth and related environmental sciencesMathematicsJournal of the Atmospheric Sciences
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